| MUHL-Music History & Lit |
| NR |
12327 |
MUHL |
1610 |
001 |
24M |
2.000 |
The World of Music |
MW |
09:10 am-10:05 am |
100 |
42 |
58 |
0 |
0 |
0 |
Stephen M Shearon (P) |
01/17-05/04 |
WMB 173 |
Credit from 4-Year College |
| NR |
13781 |
MUHL |
1610 |
002 |
24M |
2.000 |
The World of Music |
MW |
12:40 pm-01:35 pm |
30 |
18 |
12 |
0 |
0 |
0 |
Joshua A Zarbo (P) |
01/17-05/04 |
SFA 301 |
Credit from 4-Year College |
| NR |
12151 |
MUHL |
3010 |
001 |
24M |
3.000 |
History of Western Art Music I |
MWF |
08:00 am-08:55 am |
30 |
12 |
18 |
0 |
0 |
0 |
Stephen M Shearon (P) |
01/17-05/04 |
SFA 303 |
Credit from 4-Year College and Upper-Division Work |
| NR |
12152 |
MUHL |
3020 |
001 |
24M |
3.000 |
History of Western Art Music II |
MWF |
09:10 am-10:05 am |
30 |
19 |
11 |
0 |
0 |
0 |
Joseph Edward Morgan (P) |
01/17-05/04 |
SFA 211 |
Credit from 4-Year College and Upper-Division Work |
| NR |
11524 |
MUHL |
3670 |
001 |
24M |
3.000 |
History of Popular Music in America |
TR |
02:40 pm-04:05 pm |
30 |
29 |
1 |
0 |
0 |
0 |
Gregory Nathan Reish (P) |
01/17-05/04 |
SFA 303 |
Credit from 4-Year College and Upper-Division Work |
| NR |
13590 |
MUHL |
3670 |
002 |
24M |
3.000 |
History of Popular Music in America |
TR |
04:20 pm-05:45 pm |
33 |
14 |
19 |
0 |
0 |
0 |
Patrick Collins Atwater (P) |
01/17-05/04 |
SFA 301 |
Credit from 4-Year College and Upper-Division Work |
| NR |
13591 |
MUHL |
3910 |
001 |
24M |
3.000 |
Styles and Analysis of Jazz |
MWF |
12:40 pm-01:35 pm |
25 |
5 |
20 |
30 |
6 |
24 |
Don J Aliquo (P) |
01/17-05/04 |
SFA 211 |
Credit from 4-Year College and Upper-Division Work |
| NR |
11525 |
MUHL |
4060 |
001 |
24M |
3.000 |
Survey of Guitar Literature |
TR |
04:20 pm-05:45 pm |
5 |
1 |
4 |
10 |
2 |
8 |
William E Yelverton (P) |
01/17-05/04 |
SFA 211 |
Credit from 4-Year College and Upper-Division Work |
| NR |
17070 |
MUHL |
4630 |
001 |
24M |
3.000 |
Seventeenth- and Eighteenth-Century Music |
M |
04:30 pm-07:30 pm |
25 |
6 |
19 |
30 |
9 |
21 |
Joseph Edward Morgan (P) |
01/17-05/04 |
SFA 208 |
Credit from 4-Year College and Upper-Division Work |
| NR |
15804 |
MUHL |
4660 |
001 |
24M |
3.000 |
American Music |
TR |
02:40 pm-04:05 pm |
25 |
5 |
20 |
0 |
0 |
0 |
Stephen M Shearon (P) |
01/17-05/04 |
SFA 208 |
Credit from 4-Year College and Upper-Division Work |
| NR |
17045 |
MUHL |
4840 |
001 |
24M |
3.000 |
Musical Theater History |
MW |
12:40 pm-02:05 pm |
10 |
9 |
1 |
30 |
23 |
7 |
Kristi Charline Shamburger (P) |
01/17-05/04 |
BDA 218 |
Credit from 4-Year College and Upper-Division Work |
| NR |
14609 |
MUHL |
5060 |
001 |
24M |
3.000 |
Guitar Literature |
TR |
04:20 pm-05:45 pm |
5 |
1 |
4 |
10 |
2 |
8 |
William E Yelverton (P) |
01/17-05/04 |
SFA 211 |
|
| NR |
12083 |
MUHL |
5070 |
D01 |
24M |
3.000 |
Music History Survey |
|
TBA |
25 |
8 |
17 |
0 |
0 |
0 |
Stephen M Shearon (P) |
01/17-05/04 |
TBA TBA |
Distance Learning and Distance Education Fee-GR |
| NR |
17071 |
MUHL |
5630 |
001 |
24M |
3.000 |
Seventeenth and Eighteenth Century Music |
M |
04:30 pm-07:30 pm |
5 |
3 |
2 |
30 |
9 |
21 |
Joseph Edward Morgan (P) |
01/17-05/04 |
SFA 208 |
|


Subscribed users
{{users}}
TrendingInNaija
Sorry cannot load trends at the moment.
| Topic | Discussions |
|---|---|
| {{trend}} | {{trends[trend].tweet_volume}} |
About and Author
TrendingInNaija will inform you on discussions trending in Nigeria. Data is gotten from twitter
App created by Tasiu KwaplongFacebook GitHub<PHONE_NUMBER>6


AL-01 AL-02 AL-03 AL-04 AL-05 AL-06 AL-07
AL – Sen. Richard C. Shelby (R) and Sen. Doug Jones (D)
Committees
Richard C. Shelby is the #10 Republican on the Senate Appropriations Subcommittee on Commerce, Justice, Science, and Related Agencies
Richard C. Shelby is the #1 Republican on the Senate Committee on Appropriations
Richard C. Shelby is the #3 Republican on the Senate Appropriations Subcommittee on Energy and Water Development
HEP Grants
In the past 9 years, this state has received: 17 HEP grants, totalling $5,383,000
Year Institution Amount ($)
------ ---------------------------------- ------------
2019 University of Alabama 674,000
2019 University of Alabama - Birmingham 348,000
2018 University of Alabama 666,000
2018 University of Alabama - Birmingham 345,000
2017 University of Alabama 653,000
2017 University of Alabama - Birmingham 367,000
2016 University of Alabama 485,000
2015 University of Alabama 585,000
2014 University of Alabama 505,000
2013 University of Alabama 275,000
2013 University of South Alabama 0
2012 University of Alabama 410,000
2012 University of South Alabama 70,000
SC Contracts
This state received no SC contracts from 2012-2020
NSF MPS Grants
In the past 9 years, this state has received: 209 NSF MPS grants, totalling $37,628,106
Institution Amount ($)
----------------------------------- ------------
University Of Alabama 10,937,975
Auburn University 9,396,709
University Of Alabama At Birmingham 8,853,090
Tuskegee University 3,861,873
University Of Alabama In Huntsville 1,482,872
Alabama A & M University 1,401,010
University Of South Alabama 697,471
University Of Alabama Birmingham 652,189
Alabama State University 271,535
University Of North Alabama 48,544
Troy University 24,838
SULI/CCI Interns
From 2014-2018, this state had 57 SULI/CCI interns
# Interns Program College
----------- --------- ----------------------------------------------
16 SULI Auburn University
12 SULI The University of Alabama
7 SULI University of Alabama at Birmingham
7 SULI University of Alabama in Huntsville
6 SULI Alabama Agricultural and Mechanical University
2 SULI Birmingham-Southern College
2 SULI Tuskegee University
1 CCI J.F. Drake State Technical College
1 SULI Alabama State University
1 SULI Auburn University at Montgomery
1 SULI Troy University
1 SULI University of South Alabama
57 — — Back to top
AL-01 – Rep. Bradley Byrne (R) – Wikipedia
HEP Grants
In the past 9 years, this district has received: $70,000 in SC HEP grants.
Institution Amount ($) Start End Principal Investigator Project Title
--------------------------- ------------ ------- ----- ------------------------ -------------------------------------------------------------------------------------------------------------------------------
University of South Alabama 70000 2012 2014 Jenkins Experimental High Energy Physics at the University of South Alabama: Request to Continue Activities for CMS, BaBaR and Belle II
SC Contracts
This district received no SC contracts from 2012-2020
NSF MPS Grants
In the past 9 years, this district has received: $697,471 in NSF MPS grants.
Year Institution Amount ($)
------ --------------------------- ------------
2019 University Of South Alabama 72,471
2018 University Of South Alabama 330,000
2017 University Of South Alabama 10,000
2015 University Of South Alabama 285,000
SULI/CCI Interns
From 2014-2018, this district had 1 SULI/CCI intern
Term Name College Host Lab Program
----------- --------------- --------------------------- ------------------------------ ---------
Summer 2016 Danielle Adamek University of South Alabama Brookhaven National Laboratory SULI
AL-02 – Rep. Martha Roby (R) – Wikipedia
Committees
Martha Roby is the #2 Republican on the House Appropriations Subcommittee on Commerce, Justice, and Science
Martha Roby is the #16 Republican on the House Committee on Appropriations
HEP Grants
This district received no SC HEP grants from 2012-2020
SC Contracts
This district received no SC contracts from 2012-2020
NSF MPS Grants
In the past 9 years, this district has received: $660,406 in NSF MPS grants.
Year Institution Amount ($)
------ ------------------------ ------------
2019 Auburn University 226,211
2019 Troy University 18,621
2018 Troy University 6,217
2016 Alabama State University 271,535
2015 Auburn University 137,822
SULI/CCI Interns
From 2014-2018, this district had 2 SULI/CCI interns
Term Name College Host Lab Program
----------- -------------------------- ------------------------------- -------------------------------------- ---------
Summer 2018 Ernest Sebastian Keola Lee Troy University Brookhaven National Laboratory SULI
Spring 2018 Manal Abdalla Auburn University at Montgomery Lawrence Livermore National Laboratory SULI
AL-03 – Rep. Mike Rogers (R) – Wikipedia
HEP Grants
This district received no SC HEP grants from 2012-2020
SC Contracts
This district received no SC contracts from 2012-2020
NSF MPS Grants
In the past 9 years, this district has received: $12,894,549 in NSF MPS grants.
Year Institution Amount ($)
------ ------------------- ------------
2020 Auburn University 128,291
2019 Auburn University 648,976
2019 Tuskegee University 425,000
2018 Auburn University 2,699,546
2018 Tuskegee University 1,288,750
2017 Auburn University 1,363,650
2017 Tuskegee University 778,449
2016 Auburn University 1,651,178
2015 Auburn University 315,492
2015 Tuskegee University 507,374
2014 Auburn University 1,132,896
2014 Tuskegee University 862,300
2013 Auburn University 587,586
2012 Auburn University 505,061
SULI/CCI Interns
From 2014-2018, this district had 18 SULI/CCI interns
Term Name College Host Lab Program
----------- ------------------------- ------------------- ---------------------------------------------- ---------
Summer 2018 Jonathan Carroll Auburn University Thomas Jefferson National Accelerator Facility SULI
Summer 2018 Madeline Elizabeth Dueitt Auburn University Lawrence Berkeley National Laboratory SULI
Summer 2018 Justin Thomas Smith Auburn University Brookhaven National Laboratory SULI
Summer 2018 Kaitlyn Leigh Lawrence Auburn University Oak Ridge National Laboratory SULI
Summer 2018 Jonathan Henry Phillips Tuskegee University Lawrence Berkeley National Laboratory SULI
Summer 2018 Jonathan Andrew Gonzalez Auburn University Lawrence Berkeley National Laboratory SULI
Summer 2018 Haley Barone Alix Auburn University Brookhaven National Laboratory SULI
Summer 2017 Ayden Joseph Kish Auburn University Princeton Plasma Physics Laboratory SULI
Summer 2017 Eartha Leann Thompson Tuskegee University Oak Ridge National Laboratory SULI
Summer 2016 Matthew Barry Auburn University Princeton Plasma Physics Laboratory SULI
Summer 2016 Zechun Yang Auburn University Brookhaven National Laboratory SULI
Summer 2016 Matthew David Preisser Auburn University Pacific Northwest National Laboratory SULI
Summer 2015 Matthew Barry Auburn University SLAC National Accelerator Laboratory SULI
Summer 2014 Brittany Margaret Sipin Auburn University Oak Ridge National Laboratory SULI
Summer 2014 Robert Joseph Joseph Auburn University Oak Ridge National Laboratory SULI
Spring 2017 Jonathan Andrew Gonzalez Auburn University National Renewable Energy Laboratory SULI
Fall 2018 Elizabeth Prior Auburn University Oak Ridge National Laboratory SULI
Fall 2014 Daniel Dario Martinez Auburn University Lawrence Berkeley National Laboratory SULI
AL-04 – Rep. Robert B. Aderholt (R) – Wikipedia
Committees
Robert B. Aderholt is the #1 Republican on the House Appropriations Subcommittee on Commerce, Justice, and Science
Robert B. Aderholt is the #3 Republican on the House Committee on Appropriations
HEP Grants
This district received no SC HEP grants from 2012-2020
SC Contracts
This district received no SC contracts from 2012-2020
NSF MPS Grants
This district received no NSF MPS grants from 2012-2020
SULI/CCI Interns
This district had no SULI/CCI interns from 2014-2018
AL-05 – Rep. Mo Brooks (R) – Wikipedia
Committees
Mo Brooks is the #2 Republican on the House Committee on Science, Space, and Technology
HEP Grants
This district received no SC HEP grants from 2012-2020
SC Contracts
This district received no SC contracts from 2012-2020
NSF MPS Grants
In the past 9 years, this district has received: $2,932,426 in NSF MPS grants.
Year Institution Amount ($)
------ ----------------------------------- ------------
2020 University Of Alabama In Huntsville 35,000
2019 Alabama A & M University 45,000
2018 University Of Alabama In Huntsville 145,847
2018 Alabama A & M University 716,058
2017 University Of Alabama In Huntsville 588,304
2017 Alabama A & M University 137,431
2016 Alabama A & M University 124,741
2015 University Of Alabama In Huntsville 198,343
2015 Alabama A & M University 159,280
2014 University Of Alabama In Huntsville 60,172
2014 Alabama A & M University 89,000
2013 University Of North Alabama 29,430
2013 University Of Alabama In Huntsville 84,929
2013 Alabama A & M University 89,000
2012 University Of Alabama In Huntsville 370,277
2012 University Of North Alabama 19,114
2012 Alabama A & M University 40,500
SULI/CCI Interns
From 2014-2018, this district had 14 SULI/CCI interns
Term Name College Host Lab Program
----------- -------------------- ---------------------------------------------- ------------------------------ ---------
Summer 2018 Jacob Kunisch University of Alabama in Huntsville Argonne National Laboratory SULI
Summer 2017 Lauren Walker Alabama Agricultural and Mechanical University Oak Ridge National Laboratory SULI
Summer 2017 Derek Mitchell University of Alabama in Huntsville Oak Ridge National Laboratory SULI
Summer 2017 Tiia Vesalainen University of Alabama in Huntsville Oak Ridge National Laboratory SULI
Summer 2016 Rachel Sanders Alabama Agricultural and Mechanical University Brookhaven National Laboratory SULI
Summer 2016 Lauren Walker Alabama Agricultural and Mechanical University Brookhaven National Laboratory SULI
Summer 2016 William Blake Hawley University of Alabama in Huntsville Oak Ridge National Laboratory SULI
Summer 2015 Renee Chan University of Alabama in Huntsville Brookhaven National Laboratory SULI
Summer 2014 john mwathi Alabama Agricultural and Mechanical University Brookhaven National Laboratory SULI
Summer 2014 Michael Avery Knotts Alabama Agricultural and Mechanical University Oak Ridge National Laboratory SULI
Summer 2014 Shaun Perryman J.F. Drake State Technical College Oak Ridge National Laboratory CCI
Spring 2016 Daniel Smallwood University of Alabama in Huntsville Oak Ridge National Laboratory SULI
Spring 2015 William Blake Hawley University of Alabama in Huntsville Oak Ridge National Laboratory SULI
Spring 2014 Belther Monono Alabama Agricultural and Mechanical University Oak Ridge National Laboratory SULI
AL-06 – Rep. Gary J. Palmer (R) – Wikipedia
HEP Grants
This district received no SC HEP grants from 2012-2020
SC Contracts
This district received no SC contracts from 2012-2020
NSF MPS Grants
This district received no NSF MPS grants from 2012-2020
SULI/CCI Interns
From 2014-2018, this district had 7 SULI/CCI interns
Term Name College Host Lab Program
----------- ------------------------ ----------------------------------- ------------------------------------- ---------
Summer 2018 Karly Casey University of Alabama at Birmingham Brookhaven National Laboratory SULI
Summer 2017 Joanna Schmidt University of Alabama at Birmingham Los Alamos National Laboratory SULI
Summer 2016 Kristina Celeste Fong University of Alabama at Birmingham Brookhaven National Laboratory SULI
Summer 2016 Aidan O'beirne University of Alabama at Birmingham Los Alamos National Laboratory SULI
Summer 2015 Kristina Celeste Fong University of Alabama at Birmingham Brookhaven National Laboratory SULI
Summer 2015 Luke Mitchell McClintock University of Alabama at Birmingham Los Alamos National Laboratory SULI
Spring 2016 Joshua Josiah Pritchett University of Alabama at Birmingham Lawrence Berkeley National Laboratory SULI
AL-07 – Rep. Terri A. Sewell (D) – Wikipedia
HEP Grants
In the past 9 years, this district has received: $5,313,000 in SC HEP grants.
Institution Amount ($) Start End Principal Investigator Project Title
---------------------------------- ------------ ------- ----- ------------------------ ------------------------------------------------------------------------------------------------------
University of Alabama - Birmingham 1,060,000 2017 2020 Mirov, Sergey Novel, Middle and Long Wave Infrared Lasers For Particle Accelerator and X-ray Generation Applications
University of Alabama 120,000 2015 2017 Okada, Nobuchika Research in Theoretical High Energy Physics
University of Alabama 3,448,000 2014 2020 Busenitz, Jerome Research in Elementary Particle Physics
University of Alabama 635,000 2012 2014 Busenitz Research in Neutrino Physics
University of Alabama 50,000 2012 2013 Okada Research in Theoretical High Energy Physics
SC Contracts
This district received no SC contracts from 2012-2020
NSF MPS Grants
In the past 9 years, this district has received: $20,443,254 in NSF MPS grants.
Year Institution Amount ($)
------ ----------------------------------- ------------
2020 University Of Alabama 369,288
2019 University Of Alabama At Birmingham 1,878,743
2019 University Of Alabama 1,417,487
2018 University Of Alabama At Birmingham 1,170,762
2018 University Of Alabama 1,497,759
2017 University Of Alabama At Birmingham 1,083,885
2017 University Of Alabama 541,526
2016 University Of Alabama At Birmingham 1,772,912
2016 University Of Alabama 653,761
2015 University Of Alabama Birmingham 652,189
2015 University Of Alabama At Birmingham 771,862
2015 University Of Alabama 1,517,934
2014 University Of Alabama At Birmingham 711,592
2014 University Of Alabama 1,134,870
2013 University Of Alabama At Birmingham 753,080
2013 University Of Alabama 1,600,098
2012 University Of Alabama At Birmingham 710,254
2012 University Of Alabama 2,205,252
SULI/CCI Interns
From 2014-2018, this district had 15 SULI/CCI interns
Term Name College Host Lab Program
----------- ---------------------------- --------------------------- ------------------------------------- ---------
Summer 2018 Zach Macintyre The University of Alabama Oak Ridge National Laboratory SULI
Summer 2018 Margot Blaire Woolverton Birmingham-Southern College Oak Ridge National Laboratory SULI
Summer 2017 Daryl Lakner The University of Alabama Argonne National Laboratory SULI
Summer 2016 Travis Taylor The University of Alabama Oak Ridge National Laboratory SULI
Summer 2016 Emma Clements The University of Alabama National Renewable Energy Laboratory SULI
Summer 2016 Matthew Fister The University of Alabama Los Alamos National Laboratory SULI
Summer 2015 Zachary Thane Thompson The University of Alabama Oak Ridge National Laboratory SULI
Summer 2014 Laurel Johnson The University of Alabama Argonne National Laboratory SULI
Summer 2014 Barry Clay Burrows The University of Alabama Oak Ridge National Laboratory SULI
Summer 2014 Trisha D. Handley Alabama State University Ames National Laboratory SULI
Summer 2014 Jake Farell The University of Alabama Savannah River National Laboratory SULI
Spring 2015 Marissa Amey Jenness Leshnov The University of Alabama National Renewable Energy Laboratory SULI
Fall 2018 Jared Horner The University of Alabama Oak Ridge National Laboratory SULI
Fall 2015 Kaitlyn Leigh Somazze The University of Alabama Idaho National Laboratory SULI
Fall 2014 Huda Qureshi Birmingham-Southern College Lawrence Berkeley National Laboratory SULI


your tagline here
Sorry, there was a problem with handling your request.
Copyright © 2007-2012 | Powered by SilverStripe Open Source CMS


22 showstopping looks from the Miss Universe pageant over the years, Business Insider - Business Insider Singapore
by Sophia Mitrokostas- The Miss Universe beauty pageant has been happening since 1952.
- Each year, contestants wear glamorous gowns, shimmering swimsuits, and other looks to impress the judges.
- The most glamorous looks from competitors reflect changing fashions throughout the decades.
- Visit Insider’s homepage for more stories.
In the world of pageants, the Miss Universe competition is the pinnacle of achievement, which means the fashions featured in it are no joke.
From skin-tight swimwear to elaborate ball gowns, pageant hopefuls have paraded their most showstopping looks across the Miss Universe stage since 1952.
Here’s a peek at some of the most memorable styles from the past few decades.
Miss Argentina 2019 competed in this shimmery, angelic look.
Mariana Jesica Varela, Miss Argentina 2019, turned heads in this glittering, beaded outfit that was complete with a feathery attachment a large, spiked crown.
In 2019, Shweta Sekhon wore an over-the-top ensemble complete with a table.
Shweta Sekhon, who competed as Miss Malaysia in the 2019 Miss Universe competition, paid tribute to Malaysia’s Peranakan culture with this national costume.
Catriona Gray of the Philippines appeared onstage in a striking red gown before her 2018 Miss Universe win.
Catriona Gray won the 2018 Miss Universe title after appearing in mesmerizing red dress with galactic vibes.
The gown featured a plunging asymmetrical neckline and was accessorized with sparkly earrings and a bold red lip.
Iris Mittenaere of France was crowned in 2017 while wearing a form-fitting gold gown.
Iris Mittenaere accepted her title in a sparkling gold gown with long sleeves and geometric detailing. She is now a TV host and actress.
Olivia Culpo represented US as the winner of the 2012 Miss Universe pageant.
Before she was a fashion influencer and actress, Olivia Culpo wowed pageant judges in a brilliant magenta gown during her 2012 Miss Universe win.
She skipped jewelry for this look, allowing the dramatic dress to take center stage.
Leila Lopes of Angola won the Miss Universe title in a head-turning feathered dress.
Leila Lopes wowed audiences with a sleeveless white gown trimmed in feathery strands. She opted for a strapless neckline and small, sparkling earrings to complete the look.
She has also gone on to star in a number of films and host TV shows.
Dayana Mendoza was crowned Miss Universe 2008 in a yellow dress.
Dayana Mendoza, who was Miss Venezuela 2008, was crowned Miss Universe 2008 while wearing a strapless yellow gown that was covered in beading.
Mendoza went on to star in a number of films.
Miss Universe 2006 wore one of the most daring looks in the pageant that year.
Zuleyka Rivera Mendoza of Puerto Rico was crowned Miss Universe 2006 while wearing this nearly see-through metallic dress that looks like it’s made of magical chains.
Mendoza went on to become a TV host, dancer, and actress.
Jennifer Hawkins of Australia was crowned in 2004 while wearing a detailed gold gown.
Jennifer Hawkins appeared on stage wearing a textured golden dress accessorized with a sparkling bracelet and dramatic statement necklace.
The pageant queen would go on to work as a fashion designer and model, appearing on the covers of magazines like Elle, Harper’s Bazaar, Cosmopolitan, and Maxim.
Lara Dutta of India became the first Miss Universe of the new millennium, wearing a slinky red dress.
Her gown featured a modern one-shoulder design and a curve-hugging cut. Lara Dutta paired the dress with a matching red wrap.
Dutta has been in a number of Hindi films and has won awards for her work.
Mpule Kwelagobe competed in an elegant, off-the-shoulder gown in 1999.
Representing Botswana, Mpule Kwelagobe was crowned Miss Universe 1999 in this regal champagne-colored gown with rhinestone details.
Kwelagobe went on to become the CEO of her own company, the Mpule Foundation.
Sushmita Sen turned heads in a daring black gown when she was crowned in 1994.
Sushmita Sen became the first woman from India to win the Miss Universe title – and she wore a black gown with gold fringe and detailing to pose with her crown.
Angela Visser, Miss Universe 1989, posed in a perfectly draped gown.
Angela Visser looked radiant in a floor-length evening gown decorated with sparkling sequined scales.
She was just 22 years old when she was crowned.
Miss Universe 1987 has donned a sequined evening gown.
Cecilia Bolocco of Chile stunned in a sleeveless gown that featured a cascade of white and gold sequined feathers.
After her Miss Universe win, Cecilia Bolocco went on to work as a journalist for CNN.
Irene Saez of Venezuela modeled a memorable national costume during the pageant.
Miss Universe 1981 Irene Saez was surrounded by ruffles as she showed off the jaw-dropping pink and white dress that’s edged with lace. Her hair was styled in simple shoulder-length curls.
Saez went on to become a politician and was once elected governor of the state of Nueva Esparta.
Miss Universe 1973 showed off her new title in a flowing white gown.
Maria Margarita Moran of the Philippines dazzled in a long gown with cape-like shoulder embellishments and a high neckline.
She’s the second Miss Universe winner from the Philippines.
Georgina Rizk of Lebanon took home the 1971 crown in a colorful two-piece ensemble.
The pageant queen beamed as she accepted her scepter and crown in the company of Miss Puerto Rico 1970.
Georgina Rizk’s outfit was composed of a plunging top made of gauzy blue fabric and beads, along with matching silky pants and a voluminous hairstyle.
Martha Vasconcellos of Brazil stunned in a beaded gown after winning the 1968 crown.
The striking dress covered Martha Vasconcellos in head-to-toe beadwork. She accessorized with gently curled shoulder-length hair and a bright smile.
Along with her crown, Vasconcellos won prizes including a three-piece wig wardrobe and a custom kimono.
After her 1964 win, Kiriaki “Corinna” Tsopei of Greece held court in a stunning satin gown.
Kiriaki “Corinna” Tsopei beamed in a silky evening gown with beaded detailing on the shoulders.
She was the competition’s first Greek winner and went on to become a film and television actress.
Iêda Maria Vargas of Brazil shined in a detailed gown after being crowned in 1963.
The light gown perfectly complements her new fur-lined cloak. Intricate beading sparkles down the length of the dress, and the look was finished off with elbow-length evening gloves.
Vargas went on to become an actress.
Akiko Kojima of Japan wowed in a traditional outfit before winning the 1959 event.
The former Miss Japan opted to compete in a printed kimono paired with a headdress. On her feet, Akiko Kojima wore sandals and tabi, traditional Japanese split-toed socks.
Akiko Kojima was the first Japanese woman to win Miss Universe.
Miriam Stevenson won the title in 1954 in a fringed bathing suit.
Miriam Stevenson was the first Miss USA to win the Miss Universe pageant and the first titleholder to earn a college degree while holding the title.
Notably, the South Carolina native competed wearing clothing she had made herself.
- Read more:
- A 22-year-old beauty queen has been stripped of her title after getting pregnant because it reportedly goes against pageant rules
- 25 celebrities that you didn’t realize competed in beauty pageants
- Photos of the exact moment 35 contestants found out they won Miss Universe
- Here’s what 26 Miss USA contestants look like without makeup


Changeset 530 for mystic/setup.py
- Timestamp:
- 05/06/12 10:57:22 (4 years ago)
- File:
-
- 1 edited
-
mystic/setup.py (modified) (3 diffs)
Legend:
- Unmodified
- Added
- Removed
-
mystic/setup.py
r475 r530 3 3 # Michael McKerns 4 4 #<EMAIL_ADDRESS>5 6 from __future__ import with_statement 7 import os 8 9 # set version numbers 10 stable_version = '0.2a1' 11 target_version = '0.2a2' 12 is_release = False 5 13 6 14 # check if easy_install is available … … 13 21 has_setuptools = False 14 22 23 # generate version number 24 if os.path.exists('mystic/info.py'): 25 # is a source distribution, so use existing version 26 from mystic.info import this_version 27 elif stable_version == target_version: 28 # we are building a stable release 29 this_version = target_version 30 else: 31 # we are building a distribution 32 this_version = target_version + '.dev' 33 if is_release: 34 from datetime import date 35 today = "".join(date.isoformat(date.today()).split('-')) 36 this_version += "-" + today 37 38 # get the license info 39 with open('LICENSE') as file: 40 license_text = file.read() 41 42 # generate the readme text 43 long_description = \ 44 """------------------------------------------------------ 45 mystic: a simple model-independent inversion framework 46 ------------------------------------------------------ 47 48 The mystic framework provides a collection of optimization algorithms 49 and tools that allows the user to more robustly (and readily) solve 50 optimization problems. All optimization algorithms included in mystic 51 provide workflow at the fitting layer, not just access to the algorithms 52 as function calls. Mystic gives the user fine-grained power to both 53 monitor and steer optimizations as the fit processes are running. 54 55 Where possible, mystic optimizers share a common interface, and thus can 56 be easily swapped without the user having to write any new code. Mystic 57 solvers all conform to a solver API, thus also have common method calls 58 to configure and launch an optimization job. For more details, see 59 `mystic.abstract_solver`. The API also makes it easy to bind a favorite 60 3rd party solver into the mystic framework. 61 62 By providing a robust interface designed to allow the user to easily 63 configure and control solvers, mystic reduces the barrier to implementing 64 a target fitting problem as stable code. Thus the user can focus on 65 building their physical models, and not spend time hacking together an 66 interface to optimization code. 67 68 Mystic is in the early development stages, and any user feedback is 69 highly appreciated. Contact Mike McKerns [mmckerns at caltech dot edu] 70 with comments, suggestions, and any bugs you may find. A list of known 71 issues is maintained at http://dev.danse.us/trac/mystic/query. 72 73 74 Major Features 75 ============== 76 77 Mystic provides a stock set of configurable, controllable solvers with:: 78 79 - a common interface 80 - the ability to impose solver-independent bounds constraints 81 - the ability to apply solver-independent monitors 82 - the ability to configure solver-independent termination conditions 83 - a control handler yielding: [pause, continue, exit, and user_callback] 84 - ease in selecting initial conditions: [initial_guess, random] 85 - ease in selecting mutation strategies (for differential evolution) 86 87 To get up and running quickly, mystic also provides infrastructure to:: 88 89 - easily generate a fit model (several example models are included) 90 - configure and auto-generate a cost function from a model 91 - extend fit jobs to parallel & distributed resources 92 - couple models with optimization parameter constraints [COMING SOON] 93 94 95 Current Release 96 =============== 97 98 The latest stable release version is mystic-%(relver)s. You can download it here. 99 The latest stable version of mystic is always available at: 100 101 http://dev.danse.us/trac/mystic 102 103 104 Development Release 105 =================== 106 107 If you like living on the edge, and don't mind the promise 108 of a little instability, you can get the latest development 109 release with all the shiny new features at: 110 111 http://dev.danse.us/packages. 112 113 114 Installation 115 ============ 116 117 Mystic is packaged to install from source, so you must 118 download the tarball, unzip, and run the installer:: 119 120 [download] 121 $ tar -xvzf mystic-%(thisver)s.tgz 122 $ cd mystic-%(thisver)s 123 $ python setup py build 124 $ python setup py install 125 126 You will be warned of any missing dependencies and/or settings 127 after you run the "build" step above. Mystic depends on numpy 128 and sympy, so you should install them first. There are several 129 functions within mystic where scipy is used if it is available; 130 however, scipy is an optional dependency. Having matplotlib installed 131 is necessary for running several of the examples, and you should 132 probably go get it even though it's not required. Matplotlib is 133 also required by mystic's "analysis viewers". 134 135 Alternately, mystic can be installed with easy_install:: 136 137 [download] 138 $ easy_install -f . mystic 139 140 For Windows users, source code and examples are available in zip format. 141 A binary installer is also provided:: 142 143 [download] 144 [double-click] 145 146 147 Requirements 148 ============ 149 150 Mystic requires:: 151 152 - python, version >= 2.5, version < 3.0 153 - numpy, version >= 1.0 154 - sympy, version >= 0.6.7 155 156 Optional requirements:: 157 158 - setuptools, version >= 0.6 159 - matplotlib, version >= 0.91 160 - scipy, version >= 0.6.0 161 - pathos, version >= 0.2a.dev 162 - pyina, version >= 0.2a.dev 163 164 165 Usage Notes 166 =========== 167 168 Probably the best way to get started is to look at a few of the 169 examples provided within mystic. See `mystic.examples` for a 170 set of scripts that demonstrate the configuration and launching of 171 optimization jobs for one of the sample models in `mystic.models`. 172 Many of the included examples are standard optimization test problems. 173 174 Instructions on building a new model are in `mystic.models.abstract_model`. 175 Mystic provides base classes for two types of models:: 176 177 - AbstractFunction [evaluates f(x) for given evaluation points x] 178 - AbstractModel [generates f(x,p) for given coefficients p] 179 180 It is, however, not necessary to use the base classes in your own model. 181 Mystic also provides some convienence functions to help you build a 182 model instance and a cost function instance on-the-fly. For more 183 information, see `mystic.mystic.forward_model`. 184 185 All mystic solvers are highly configurable, and provide a robust set of 186 methods to help customize the solver for your particular optimization 187 problem. For each solver, a minimal interface is also provided for users 188 who prefer to configure their solvers in a single function call. For more 189 information, see `mystic.mystic.abstract_solver` for the solver API, and 190 each of the individual solvers for their minimal (non-API compliant) 191 interface. 192 193 Mystic extends the solver API to parallel computing by providing a solver 194 class that utilizes the parallel map-reduce algorithm. Mystic includes 195 a set of defaults in `mystic.mystic.python_map` that mirror the behavior 196 of serial python and the built-in python map function. Mystic solvers 197 built on map-reduce can utilize the distributed and parallel tools provided 198 by the `pathos` package, and thus with little new code solvers are 199 extended to high-performance computing. For more information, see 200 `mystic.mystic.abstract_map_solver`, `mystic.mystic.abstract_nested_solver`, 201 and the pathos documentation at http://dev.danse.us/trac/pathos. 202 203 Important classes and functions are found here:: 204 205 - mystic.mystic.solvers [solver optimization algorithms] 206 - mystic.mystic.termination [solver termination conditions] 207 - mystic.mystic.strategy [solver population mutation strategies] 208 - mystic.mystic.monitors [optimization monitors] 209 - mystic.mystic.tools [function wrappers, etc] 210 - mystic.mystic.forward_model [cost function generator] 211 - mystic.models [a collection of standard models] 212 - mystic.math [some mathematical functions and tools] 213 214 Solver and model API definitions are found here:: 215 216 - mystic.mystic.abstract_solver [the solver API definition] 217 - mystic.mystic.abstract_map_solver [the parallel solver API] 218 - mystic.mystic.abstract_nested_solver [the nested solver API] 219 - mystic.models.abstract_model [the model API definition] 220 221 222 License 223 ======= 224 225 Mystic is distributed under a modified BSD license. 226 227 >>> import mystic 228 >>> print mystic.license() 229 230 231 Citation 232 ======== 233 234 If you use mystic to do research that leads to publication, 235 we ask that you acknowledge use of mystic by citing the 236 following in your publication:: 237 238 M.M. McKerns, L. Strand, T. Sullivan, A. Fang, M.A.G. Aivazis, 239 "Building a framework for predictive science", Proceedings of 240 the 10th Python in Science Conference, 2011; 241 http://arxiv.org/pdf/1202.1056 242 243 Michael McKerns, Patrick Hung, and Michael Aivazis, 244 "mystic: a simple model-independent inversion framework", 2009- ; 245 http://dev.danse.us/trac/mystic 246 247 248 More Information 249 ================ 250 251 Please see http://dev.danse.us/trac/mystic or http://arxiv.org/pdf/1202.1056 for further information. 252 253 """ % {'relver' : stable_version, 'thisver' : this_version} 254 255 # write readme file 256 with open('README', 'w') as file: 257 file.write(long_description) 258 259 # generate 'info' file contents 260 def write_info_py(filename='mystic/info.py'): 261 contents = """# THIS FILE GENERATED FROM SETUP.PY 262 this_version = '%(this_version)s' 263 stable_version = '%(stable_version)s' 264 readme = '''%(long_description)s''' 265 license = '''%(license_text)s''' 266 """ 267 with open(filename, 'w') as file: 268 file.write(contents % {'this_version' : this_version, 269 'stable_version' : stable_version, 270 'long_description' : long_description, 271 'license_text' : license_text }) 272 return 273 274 # write info file 275 write_info_py() 276 15 277 # build the 'setup' call 16 278 setup_code = """ 17 279 setup(name='mystic', 18 version=' 0.2a2.dev',280 version='%s', 19 281 description='a simple interactive inversion analysis framework', 282 long_description = '''%s''', 20 283 author = 'Mike McKerns', 21 284 maintainer = 'Mike McKerns', … … 31 294 package_dir = {'mystic':'mystic','mystic.models':'models', 32 295 'mystic.math':'_math'}, 33 """ 296 """ % (target_version, long_description) 34 297 35 298 # add dependencies
Note: See TracChangeset
for help on using the changeset viewer.


What is EOS?
EOS is the most scalable, divisible, and programmable digital currency on the market.
The EOS Currency runs on the World's largest public blockchain based upon the EOSIO software platform. EOSIO is a Delegated Proof of Stake (DPoS) network where the stake-holders have the authority to select block producers / node operators. This distributes power amongst the token holders, instead of concentrating the power in the hands of the block miners, and therefore aligns the interests of all parties involved.
New to EOS? Start Here...


Just another FGO Servant Checklist, but with NP Count. I'm gonna try my best to update the list ASAP.


public class RotatableRectangle
extends java.lang.Object
| Modifier and Type | Field and Description |
|---|---|
private java.util.ArrayList<java.awt.Point> |
corners |
private int |
numberOfPoints |
private java.awt.Point |
pivot |
| Constructor and Description |
|---|
RotatableRectangle(java.util.ArrayList<java.awt.Point> points,
java.awt.Point pivot)
Constructor
Size of the points array need to be exactly four.
|
RotatableRectangle(double x,
double y,
double width,
double height)
Constructor
|
RotatableRectangle(double x,
double y,
double width,
double height,
java.awt.Point pivot)
Constructor
|
RotatableRectangle(java.awt.Point leftTop,
java.awt.Point rightTop,
java.awt.Point rightBottom,
java.awt.Point leftBottom)
Constructor
|
RotatableRectangle(java.awt.Point leftTop,
java.awt.Point rightTop,
java.awt.Point rightBottom,
java.awt.Point leftBottom,
java.awt.Point pivot)
Constructor
|
| Modifier and Type | Method and Description |
|---|---|
boolean |
contains(double x,
double y)
Used to check if a point is in this (rotated) rectangle or not.
|
boolean |
contains(int x,
int y)
Used to check if a point is in this (rotated) rectangle or not.
|
boolean |
contains(java.awt.Point point)
Used to check if a point is in this (rotated) rectangle or not.
|
double[] |
getXCoordinates()
Used to get the x positions of the corners after a rotation.
|
double[] |
getYCoordinates()
Used to get the y positions of the corners after a rotation.
|
boolean |
intersects(java.awt.Rectangle rect)
Used to check if a rectangle intersects with this (rotated) rectangle
|
private java.awt.Point |
rotatePoint(double angle,
java.awt.Point pointToRotate)
Used when rotating on of the corners around the center of this rectangle.
|
void |
rotateRect(double angle)
Used to rotate this rectangle for angle degrees
|
private java.util.ArrayList<java.awt.Point> corners
private java.awt.Point pivot
private int numberOfPoints
public RotatableRectangle(double x, double y, double width, double height)
x
- X Position of the recty
- Y Position of the rectwidth
- Width of the rectheight
- Height of the rectpublic RotatableRectangle(double x, double y, double width, double height, java.awt.Point pivot)
x
- X Position of the recty
- Y Position of the rectwidth
- Width of the rectheight
- Height of the rectpivot
- Center of the rectpublic RotatableRectangle(java.util.ArrayList<java.awt.Point> points, java.awt.Point pivot)
points
- Corners of the rectanglepivot
- Center of the rectpublic RotatableRectangle(java.awt.Point leftTop, java.awt.Point rightTop, java.awt.Point rightBottom, java.awt.Point leftBottom)
leftTop
- Point located at the leftTop of the rectrightTop
- Point located at the rightTop of the rectrightBottom
- Point located at the rightBottom of the rectleftBottom
- Point located at the leftBottom of the rectpublic RotatableRectangle(java.awt.Point leftTop, java.awt.Point rightTop, java.awt.Point rightBottom, java.awt.Point leftBottom, java.awt.Point pivot)
leftTop
- Point located at the leftTop of the rectrightTop
- Point located at the rightTop of the rectrightBottom
- Point located at the rightBottom of the rectleftBottom
- Point located at the leftBottom of the rectpivot
- Center of the rectpublic boolean contains(java.awt.Point point)
point
- Point to checkpublic boolean contains(int x, int y)
x
- X position of the pointy
- Y position of the pointpublic boolean contains(double x, double y)
x
- X position of the pointy
- Y position of the pointpublic boolean intersects(java.awt.Rectangle rect)
rect
- Rectangle to checkpublic void rotateRect(double angle)
angle
- Angle of the rotationpublic double[] getXCoordinates()
public double[] getYCoordinates()
private java.awt.Point rotatePoint(double angle, java.awt.Point pointToRotate)
angle
- Angle of the rotationpointToRotate
- Point that gets rotated


| Opcode | Instruction | Op/En | 64-Bit Mode | Compat/Leg Mode | Description |
|---|---|---|---|---|---|
| 99 | CWD | ZO | Valid | Valid | DX:AX ← sign-extend of AX. |
| 99 | CDQ | ZO | Valid | Valid | EDX:EAX ← sign-extend of EAX. |
| REX.W + 99 | CQO | ZO | Valid | N.E. | RDX:RAX← sign-extend of RAX. |
| Op/En | Operand 1 | Operand 2 | Operand 3 | Operand 4 |
| ZO | NA | NA | NA | NA |
Doubles the size of the operand in register AX, EAX, or RAX (depending on the operand size) by means of sign extension and stores the result in registers DX:AX, EDX:EAX, or RDX:RAX, respectively. The CWD instruction copies the sign (bit 15) of the value in the AX register into every bit position in the DX register. The CDQ instruction copies the sign (bit 31) of the value in the EAX register into every bit position in the EDX register. The CQO instruction (available in 64-bit mode only) copies the sign (bit 63) of the value in the RAX register into every bit position in the RDX register.
The CWD instruction can be used to produce a doubleword dividend from a word before word division. The CDQ instruction can be used to produce a quadword dividend from a doubleword before doubleword division. The CQO instruction can be used to produce a double quadword dividend from a quadword before a quadword division.
The CWD and CDQ mnemonics reference the same opcode. The CWD instruction is intended for use when the operand-size attribute is 16 and the CDQ instruction for when the operand-size attribute is 32. Some assemblers may force the operand size to 16 when CWD is used and to 32 when CDQ is used. Others may treat these mnemonics as synonyms (CWD/CDQ) and use the current setting of the operand-size attribute to determine the size of values to be converted, regardless of the mnemonic used.
In 64-bit mode, use of the REX.W prefix promotes operation to 64 bits. The CQO mnemonics reference the same opcode as CWD/CDQ. See the summary chart at the beginning of this section for encoding data and limits.
IF OperandSize = 16 (* CWD instruction *) THEN DX ← SignExtend(AX); ELSE IF OperandSize = 32 (* CDQ instruction *) EDX ← SignExtend(EAX); FI; ELSE IF 64-Bit Mode and OperandSize = 64 (* CQO instruction*) RDX ← SignExtend(RAX); FI; FI;
None
#UD If the LOCK prefix is used.


RT @jbcnconf: Announcing @kittylyst and his talk "Do We Really Do Functional Programming in Java?". Ben will talk about what FP really is,…
7/15/2021, 2:26:56 PM
Favs: 0
Retweets: 0
link--- layout: tweet ---
RT @jbcnconf: Announcing @kittylyst and his talk "Do We Really Do Functional Programming in Java?". Ben will talk about what FP really is,…
7/15/2021, 2:26:56 PM
Favs: 0
Retweets: 0
link


|
|
The "Text to Speech" audio may be triggered in any of 3 ways:
- When the scene is loaded, using the "Event Functions":
function vh_sceneLoaded(){
//the scene begins playing, add actions here
sayText('Welcome to the virtual host text to speech',1,1,3);
}
- Using a call to the sayText() command, specifying the text:
Click here to say something!
|
|


title = "Invoice" description = "Example invoice with custom font and image embed" layout = "renatio.dynamicpdf::pdf.layouts.default" ==
via Paddle.com
John Doe
Example street 16
Warszawa, 50-100
Poland
VAT Number: PL2332213309
Paddle.com Market Ltd
Judd House 18-29 Mora Street
London, EC1V 8BT
United Kingdom
VAT Number: EU372017215
Company Number: 08172165
Customer<EMAIL_ADDRESS>Order Number / Invoice: #28542217
Billing date: 01 Sep 2020
Payment method: Visa card ending 2222
Currency: USD
| Product | Quantity | Price |
|---|---|---|
| TablePlus License Renewal | 1 | US$39.00 |
| VAT (0%) | US$0.00 | |
| YOUR ORDER | US$39.00 | |
| No VAT - Supply may be subject to reverse charge in the country of receipt |
The US$39.00 payment will appear on your bank/card statement as: PADDLE.NET* TABLEPLUS
If you have a problem with your order (e.g. don’t recognise the charge, suspect a fraudulent transaction), please visit paddle.net.


{% extends "base.html" %} {% block title %}
Medieval catalogues > SECULAR INSTITUTIONS: Hospitals, Towns, and the Professions > Saffron Walden almshouse > List of chained books, 5 August 1400
{% endif %}7 identified entries found.
All data was derived from the List of Identifications by Professor Richard Sharpe.
{% if not printing %}
A key to codes used in the List is available (opens in new tab).{% endif %}


Through the HSE Delivery guidance, a performance rating of "Green" will satisfy your regulatory authority with a compliant benchmark for managing your operational risks. HTS Compliance will support you in achieving this "Green" rated standard in compliance
We provide expert engineering services and work closely with our clients to form "intelligent" inspection solutions and to meet the diverse and increasingly challenging HSE requirements.
We have proven expertise in:
Repeated Three year contract awarded for a second term for all sites and offices within the UK & Ireland, Full set-up and implementation of cloud based inspection software "AtexInspect" Fixed Wire Periodic Inspections - Hazardous area inspections - Policy implementation
Site based fixed wire periodic inspections for office and industrial plant located within a live operational manufacturing facility Fixed Wire Periodic Inspections
Site Based periodic "Atex" inspections for Close & Visual based upon site based systems Hazardous area inspections


First, let me say that this is not the way I usually take cocaine. Typically, I take it after getting very drunk (half a bottle whisky say, which though I am a large man, a seasoned boozer, and can hold my liquor, definitely gets me completely tanked), and in dosages ranging from a quarter gram to one gram. This combination results, of course, in a state of complete gonzoism bordering on derangement.
Tonight though, I started off with about a quarter gram of coke followed by very moderate beer-drinking. I didn't really feel high. After maybe an hour I was wishing I had more cocaine, so I snorted some Dilaudid (10 mg, I'm pretty sure). This took the edge off my comedown all right, but without producing any feelings of opium-like euphoria, though with a nice but far from overwhelming body buzz. My activity throughout the evening, by the way, consisted of sitting around talking with a similarly stoned old and good friend in his apartment.
After about another hour, still feeling fairly fine—just slightly more interested in everything I thought about (from the cocaine) but duly mellow as well (from the Dilaudid)—I did another quarter gram of coke. This did get me genuinely high, though with no racing heartbeat or uncontrollable volubility, again due to the Dilaudid, I assume. About half an hour later I snorted 10 mg of Oxycontin. I'd never done it before, and knew it could be dangerous, but what with my really moderate (by my standards) alcohol intake and pretty low dosages of everything else, I thought the risk was minimal.
Well, the Oxycontin very quickly delivered the intense body buzz and euphoria you'd expect from powerful opoids. It was (and still is) extremely pleasurable, especially combined with the heightened awareness of it and absence of dopiness provided by the cocaine. I do not feel deranged at all, and absolutely in control and just generally wonderful. Added to this is the calm provided by my expectation of having a pretty mild comedown, though we'll have to see if it turns out that way. But not knowing for certain that a terrible comedown awaits me adds to my sensation of well-being.
I have a lot of experience (10 years plus) with fairly regular episodes of intense impairment from the combination of large quantities of booze and fairly normal amounts of cocaine.  The combination of smallish doses I took tonight has given me very intense pleasure, comparable to that time actually, with, as far as I know, much less risk of killing myself. Since taking the Oxycontin a couple of hours ago, I've had a bit more cocaine (which was great, despite being the last of it) and am very slowly drinking some wine. I feel content and softly, quietly exhilarated, and I must say, like I've really got my money's worth, something I rarely feel after cocaine alone.
Experience Reports are the writings and opinions of the individual authors who submit them.
Some of the activities described are dangerous and/or illegal and none are recommended by Erowid.


Throwback Thursday to Halloween 2014 when I made my own Fozzie Bear costume. I had no idea how much work it would be but it was a lot of fun.
Credit to this tutorial for helping a lot.
Pattern
OK, so first we need to get the below pattern in the correct size.
With the help of Kinko and several iterations of cutting, stapling, and modeling it on my own head I am left with this.
Looking good!
Foam
Next, I went to my local craft store and purchased craft foam similar to the one below. Using the above pattern I cut the foam. Using model glue, suitable for foam, I then glued the foam together to form the head.
Fur
With the foam head finished now I began work on the fur covering.
Using the same pattern from above I cut the fur to match the same pattern as the foam. Next I glued the fur to the foam head. Afterwards, I sewed all the seems.
Coming together!
- Lots of coffee!


How will you be purchasing?
Online Purchases can be mailed or you can print the tickets yourself
A delivery fee of $2.75 will be added for mailing tickets


- onDirectoryChange(File) - Method in interface org.apache.commons.io.monitor.FileAlterationListener
-
Directory changed Event.
- onDirectoryChange(File) - Method in class org.apache.commons.io.monitor.FileAlterationListenerAdaptor
-
Directory changed Event.
- onDirectoryCreate(File) - Method in interface org.apache.commons.io.monitor.FileAlterationListener
-
Directory created Event.
- onDirectoryCreate(File) - Method in class org.apache.commons.io.monitor.FileAlterationListenerAdaptor
-
Directory created Event.
- onDirectoryDelete(File) - Method in interface org.apache.commons.io.monitor.FileAlterationListener
-
Directory deleted Event.
- onDirectoryDelete(File) - Method in class org.apache.commons.io.monitor.FileAlterationListenerAdaptor
-
Directory deleted Event.
- ONE_EB - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in an exabyte.
- ONE_EB_BI - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in an exabyte.
- ONE_GB - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in a gigabyte.
- ONE_GB_BI - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in a gigabyte.
- ONE_KB - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in a kilobyte.
- ONE_KB_BI - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in a kilobyte.
- ONE_MB - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in a megabyte.
- ONE_MB_BI - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in a megabyte.
- ONE_PB - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in a petabyte.
- ONE_PB_BI - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in a petabyte.
- ONE_TB - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in a terabyte.
- ONE_TB_BI - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in a terabyte.
- ONE_YB - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in a yottabyte.
- ONE_ZB - Static variable in class org.apache.commons.io.FileUtils
-
The number of bytes in a zettabyte.
- onFileChange(File) - Method in interface org.apache.commons.io.monitor.FileAlterationListener
-
File changed Event.
- onFileChange(File) - Method in class org.apache.commons.io.monitor.FileAlterationListenerAdaptor
-
File changed Event.
- onFileCreate(File) - Method in interface org.apache.commons.io.monitor.FileAlterationListener
-
File created Event.
- onFileCreate(File) - Method in class org.apache.commons.io.monitor.FileAlterationListenerAdaptor
-
File created Event.
- onFileDelete(File) - Method in interface org.apache.commons.io.monitor.FileAlterationListener
-
File deleted Event.
- onFileDelete(File) - Method in class org.apache.commons.io.monitor.FileAlterationListenerAdaptor
-
File deleted Event.
- onStart(FileAlterationObserver) - Method in interface org.apache.commons.io.monitor.FileAlterationListener
-
File system observer started checking event.
- onStart(FileAlterationObserver) - Method in class org.apache.commons.io.monitor.FileAlterationListenerAdaptor
-
File system observer started checking event.
- onStop(FileAlterationObserver) - Method in interface org.apache.commons.io.monitor.FileAlterationListener
-
File system observer finished checking event.
- onStop(FileAlterationObserver) - Method in class org.apache.commons.io.monitor.FileAlterationListenerAdaptor
-
File system observer finished checking event.
- openInputStream(File) - Static method in class org.apache.commons.io.FileUtils
-
Opens a FileInputStream
for the specified file, providing better
error messages than simply calling new FileInputStream(file)
.
- openOutputStream(File) - Static method in class org.apache.commons.io.FileUtils
-
Opens a FileOutputStream
for the specified file, checking and
creating the parent directory if it does not exist.
- openOutputStream(File, boolean) - Static method in class org.apache.commons.io.FileUtils
-
Opens a FileOutputStream
for the specified file, checking and
creating the parent directory if it does not exist.
- openReadOnly(File) - Static method in class info.ata4.util.io.NIOFileUtils
-
- openReadOnly(File, int, int) - Static method in class info.ata4.util.io.NIOFileUtils
-
- openReadWrite(File) - Static method in class info.ata4.util.io.NIOFileUtils
-
- openReadWrite(File, int, int) - Static method in class info.ata4.util.io.NIOFileUtils
-
- or(IOFileFilter...) - Static method in class org.apache.commons.io.filefilter.FileFilterUtils
-
Returns a filter that ORs the specified filters.
- orFileFilter(IOFileFilter, IOFileFilter) - Static method in class org.apache.commons.io.filefilter.FileFilterUtils
-
- OrFileFilter - Class in org.apache.commons.io.filefilter
-
A FileFilter
providing conditional OR logic across a list of
file filters.
- OrFileFilter() - Constructor for class org.apache.commons.io.filefilter.OrFileFilter
-
Constructs a new instance of OrFileFilter
.
- OrFileFilter(List<IOFileFilter>) - Constructor for class org.apache.commons.io.filefilter.OrFileFilter
-
Constructs a new instance of OrFileFilter
with the specified filters.
- OrFileFilter(IOFileFilter, IOFileFilter) - Constructor for class org.apache.commons.io.filefilter.OrFileFilter
-
Constructs a new file filter that ORs the result of two other filters.
- org.apache.commons.io - package org.apache.commons.io
-
This package defines utility classes for working with streams, readers,
writers and files.
- org.apache.commons.io.comparator - package org.apache.commons.io.comparator
-
This package provides various Comparator
implementations
for File
s.
- org.apache.commons.io.filefilter - package org.apache.commons.io.filefilter
-
This package defines an interface (IOFileFilter) that combines both
FileFilter
and FilenameFilter
.
- org.apache.commons.io.input - package org.apache.commons.io.input
-
This package provides implementations of input classes, such as
InputStream
and Reader
.
- org.apache.commons.io.monitor - package org.apache.commons.io.monitor
-
This package provides a component for monitoring file system events
(directory and file create, update and delete events).
- org.apache.commons.io.output - package org.apache.commons.io.output
-
This package provides implementations of output classes, such as
OutputStream
and Writer
.


[gecode-users] memory exception
Guido Tack
tack at gecode.org
Fri Jan 22 21:59:59 CET 2010
frank lemoine wrote:
> hello gecode users,
>
> i working on a CSP problem that involve graphs nodes, from 10 to 999 nodes it's ok no problem but when i try more than 1000 nodes i've this message:
>
> Exception: memory : heap memory exhausted.
> Stopping
>
> so I wonder if there are solutions to this limitation
Increase the recomputation limits in the search engine options (or buy more memory, obviously).
Cheers,
Guido
-------------- next part --------------
An HTML attachment was scrubbed...
URL: <http://www.gecode.org/pipermail/users/attachments/20100122/ac5b6e26/attachment.htm>
More information about the users
mailing list


well, thanks for the spirited, thought-provoking discussion, gentlemen. Its time to put the kiddos to bed. I appreciate the sparring and I appreciate people who make good cases. So thanks for a fun debate. I will check back in later to see what I missed. Cheers
3


Kris Shaffer, Ph.D.
University of Mary Washington
pushpullfork.com / @krisshaffer
view presentation (with live links) at pushpullfork.com/blendedhybrid
fork presentation at github.com/kshaffer/blendedhybrid
Kris Shaffer, Ph.D.
University of Mary Washington
pushpullfork.com / @krisshaffer
view presentation (with live links) at pushpullfork.com/blendedhybrid
fork presentation at github.com/kshaffer/blendedhybrid


Established more than thirty years ago, MET’s Computer Science department remains a leader in a number of state-of-the-art IT areas, such as information security, computer networks, computer information systems, financial informatics, digital forensics, and health informatics. A regional and national leader in information security education for almost a decade, our curriculum is certified by the Committee on National Security Systems (CNSS).
Our world-class IT programs are driven by exceptional faculty whose scholarly accomplishments and unique industry experience place them among the top of their field. Adhering to the highest academic standards of BU, these dedicated scholars are involved in research projects in areas such as novel Internet architectures, smartphone applications, information assurance, and biomedical informatics
Most importantly, our professors are fully engaged with their students, following their progress, maintaining awareness of what’s going on in their lives and careers, and providing the support they need. An academic advisor is available to help students make the best decisions about classes.
Our part-time and online study options offer convenient times, locations, and delivery methods, ensuring that dedicated professionals have the opportunity to experience a rigorous academic environment while pursuing full-time careers. At the same time, we remain the first choice for a number of international students interested in the BU experience, and in continuing their academic development in computer science and information technology.
The broad range of backgrounds, interests, and experiences that characterize the Metropolitan College student body is integral to our programs. Students and faculty alike are rewarded by the exchange of ideas and full participation in learning—and to us that is extremely important and valuable. By graduation, our students have the ability to analyze problems more efficiently, and they have a prestigious credential from Boston University—their key to the doors of academia and careers in the industry.
I invite you to join us in navigating the changing landscape of modern information technology—certainly the most exciting and invigorating discipline in which to study, explore, and work
Anatoly Temkin, Ph.D. Chairman, Department of Computer Science Boston University Metropolitan College


Airlines
Name
Status
Create Date
Update Date
Edit
Aeromexico
Active
05/05/2019
10/05/2019
Edit
Agregar
New airline
×
Name
Close
Save
Edit airline
×
Name:
Status
Active
Inactive
Close
Save
Delete airline
×
Name:


Specify default Allure report Test Management System (TMS) pattern.
In this pattern, the %s placeholder will be replaced with test ID.
Default value (%s) is not taken into account and can be overridden (e.g. with JVM argument -Dallure.tests.management.pattern=%s).


Any programmer worth their weight in bitcoins is going to need to know a bit about databases. If you’re not familiar with databases, you should take some time to read up on them, but hurry back, because for this post we’re going to be talking about the different kinds of JOINS. ‘Joins’ are a method of linking multiple tables in a database together so we can access values from them with a single query. Seems simple enough, but joins can be confusing. Since tables in a database aren’t tangible things, it can be difficult to understand the links we create between them. I for one find it difficult to really wrap my head around a concept until I can draw it, which made for some interesting moments in high school sex ed, but also led me to develop a method for visualizing how the different kinds of joins work! Let’s have a look:
3 RING BINDER
Picture the two tables in our database as two pieces of looseleaf. The blue lines represent our rows, or records. The dashed lines represent our columns.
Now, using the SQL syntax for sqlite3, we’ll start writing our join by stipulating which tables we’d like to link.
1 2 |
|
We’ll go over INNER JOIN in a second, but for now just picture us putting our two pieces of looseleaf into a three ring binder. We’re selecting from both persons (left table) and orders (right table), and linking them with a join.
Now that our pages (tables) are in a binder (joined), we need to stipulate which column to link them on.
1 2 3 |
|
Here, we’re saying that we should link the rows in persons and orders based on the value of the ‘id’ column in the person table, and the ‘pid’ column in the orders table. When the values in those two columns match, we can assume a correlation between the two records.
Now we’ve joined our tables. But there are a few different ways to join two tables, which will effect which rows are returned. Let’s have a look:
Inner Join:
An inner join, or left inner join, will produce only the records for which there is a match from tablea (persons) and tableb (orders) (records produced are highlighted):
Left Outer Join:
A left outer join will produce a complete set of records for tablea (persons), with matching records from tableb (orders) when they exist. If there’s no match from tableb, the right table’s join column value will be ‘null’.
Right Outer Join:
A right outer join will produce a complete set of records for tableb (orders), with matching records from tablea (persons) when they exist. If there’s no match from tablea, the left table’s join column value will be ‘null’.
Full Outer Join:
A full outer join will produce the complete set of records from both tables. Wherever there is no match, the value will be ‘null’.
Conclusion:
Hopefully this visualization will help you wrap your head around database table joins, (and maybe conjure fond memories of decorating your Five Star™ binders…). For more on databases and visualizations for joins, you can go here, or here for some great insights.


def test_conv_deeper_stub():
model = get_conv_model()
graph = Graph(model, False)
layer_num = graph.n_layers
graph.to_conv_deeper_model(5, 3)
assert graph.n_layers == layer_num + 4
def test_conv_deeper_stub():
graph = get_conv_dense_model()
layer_num = graph.n_layers
graph.to_conv_deeper_model(5, 3)
assert graph.n_layers == layer_num + 4


4 references to IncludeArchivedCerts
Microsoft.PowerShell.Security (4)
security\CertificateProvider.cs (4)
1080
store.Open(
IncludeArchivedCerts
());
1754
store.Open(
IncludeArchivedCerts
());
2090
store.Open(
IncludeArchivedCerts
());
2437
store.Open(
IncludeArchivedCerts
());


Prediction about agriculture from machine can be more useful for Farming.
SMART AGRICULTURE is framework which provide the full API Integration and easy Installation of the system. For more details about DigiMesh Network and Its API Integration with our cloud server please refer to API Documentation.
Smart Agriculture provide the cloud services for analyzing predicting about the farms. ZigBee Newtwork is the key concept to send the data from remote area to our cloud server. We are providing Machine Learning models to predict various things in order to increase yield.
For Technical Support you can contact us here, We are happily available for details about Installation .
Due to lack of connectivity from virtual world remote areas farming could not get the scientific techniques of agriculture which can increase the production. To connect remote areas with virtual world we used many technologies & merge them to provide scientific ways of agriculture.
This was impossible to collect the farms data like Soil Moisture , Humidity , Temperature wind speed etc without using any local network. ZigBee Network cheap and easy to installed with Internet of The Things so this is the best choice to collect the farms data to some repository.
Edge computing work like a small computing in at device level like fields sensors. FOG computing is small computing for collecting the data from edge and works like intermediary between edge and cloud server.Raspberry pi can be used to for Edge and FOG to collect farms real time data and to send out cloud
.....
To Provide the best Decisions to farmer AI & Machine Learning is using. There are some issue in traditional farming farmer does not know which crop is best for that field and what is the best time of sowing.


developed a package to help writing Alfred 3 Workflows in PHP
then developed a package to handle config settings easily in Alfred 3 Workflows in PHP 😂
all of the above is the result of my will to extend one of my previous package, Alfred Time, to allow new options as well as the use of other time tracking services
working on the release of my first book for sleeplessmind.info. Cover done. Preface on the way and it'll be ready for publishing


Exercise 1.
Method: Develop a method to measure the height of your instructor (teacher, professor, etc) and make the measurement. Use that measurement to make another measurement. Then use the second measurement in an equation.
Instructions
Split up into teams of two or more.
One team gets a tape measure. Another team gets a yardstick. Still another team gets a 1-ft ruler.
Agree on how you will measure your instructor's height.
Make the measurement according to the selected approach.
Now measure the length, width, and/or height of the classroom using the instructor's height.
Calculate the volume of the classroom using the length, width, and height.
Compare the methods selected, the tools available, the individual measurements, and the result from the equation for the different groups.
Have each group identify the possible sources of error in the exercise and how they propagate.
Discuss the groups' results with respect to the five Cs explained in the text: coincidence, correlation, causation, convergence, and consensus. Which ones apply?
Extrapolate the findings to general sources of misinformation, misleading information, studies and research taken in isolation, etc.


""" Main ground-state executable script
Note:
The simulations are intended to be used by calling the package
directly via :code:`python -m adpeps ...`, as described in
:ref:`notes/start`
"""
from jax import grad, jit, vmap, value_and_grad
from jax import random
from jax.scipy.optimize import minimize
from jax.test_util import check_grads
from scipy import optimize
from yaml import safe_load, dump
import jax
import jax.numpy as np
import numpy as onp
from adpeps.ipeps.ipeps import iPEPS, iPEPS_exci
from adpeps.utils import io
from adpeps.utils.printing import print
import adpeps.ipeps.config as sim_config
[docs]def run(config_file: str):
""" Start the simulation
Args:
config_file: filename of the configuration file
"""
energies = []
gradnorms = []
def verbose(xk, step_size=None):
""" Output printing function """
try:
energies.append(obj.cached_out)
gradnorms.append(obj.gradnrm)
except:
pass
print(' ')
print(' # ======================== #')
print(' # Step completed #')
print(' # ======================== #')
print(' ')
[print(' Step %3d E: %.12f |grad|: %2.8g' % (i,E,gradnorms[i])) for i,E in enumerate(energies)]
print('\n')
# np.savez(output_file, peps=peps, v=xk, gradnorms=gradnorms, energies=energies)
print('Running')
print(config_file)
with open(config_file) as f:
cfg = safe_load(f)
# Show options
print(dump(cfg))
# Load the configuration file into the sim_config object
sim_config.from_dict(cfg)
# Initialize the iPEPS
peps = iPEPS()
output_file = io.get_gs_file()
print(f"Output file {output_file}")
if sim_config.resume and output_file.exists():
loaded_sim = np.load(output_file, allow_pickle=True)
peps = loaded_sim['peps'].item()
v = loaded_sim['v']
gradnorms = list(loaded_sim['gradnorms'])
energies = list(loaded_sim['energies'])
print("Resuming existing simulation")
verbose(v)
else:
print("Starting new simulation")
key = random.PRNGKey(sim_config.seed)
v = random.normal(key, (peps.numel(),))
v = v / np.max(np.abs(v))
obj = Objective(peps)
# Call SciPy's optimization function
obj.return_gn = False
xL = optimize.minimize(obj.out, v, method=sim_config.method, jac=obj.jac,
callback=verbose, options={'gtol': 1e-6, 'disp': True,
'maxiter':sim_config.max_iterations})
[docs]class Objective:
""" Class containing the objective function for the optimizer
"""
def __init__(self, peps: iPEPS):
"""
Args:
peps: iPEPS object to be optimized
"""
self.cached_v = None
self.cached_out = None
self.cached_jac = None
self.peps = peps
""" iPEPS object """
self.fun = peps.run
""" Objective function - CTM iterations until convergence
followed by the evaluation of the energy
"""
self.return_gn = True
@property
def gradnrm(self):
""" Norm of the gradient """
return np.linalg.norm(self.cached_jac)
[docs] def jac(self, v: np.ndarray) -> np.ndarray:
""" Computes the vector-Jacobian product (gradient) of the
iPEPS at the current point :attr:`v` in parameter space
This function is designed to work with optimizers that make separate
calls to the objective function and the gradient, by caching both.
Args:
v: input variational parameters for the site tensors of
the iPEPS
Returns:
gradient of the iPEPS with respect to the input parameters :attr:`v`
"""
# Cast the regular numpy array into a Jax numpy array for gradient tracking
v = np.array(v)
v = v / np.max(np.abs(v))
if (self.cached_jac is not None and self.cached_v is not None
and np.linalg.norm(v - self.cached_v) < 1e-14):
return self.cached_jac
# Call the forward + backward pass iPEPS code
o, g = value_and_grad(self.fun)(v)
# Convert to regular Numpy arrays so they can be passed to the optimizer
# and stored without any tracking information by Jax
o = onp.array(o)
v = onp.array(v)
g = onp.array(g)
# Cache the results
self.cached_v = v
self.cached_out = o
self.cached_jac = g
if self.return_gn:
return g, self.gradnrm
else:
return g
[docs] def out(self, v):
""" Computes the objective function (energy) of the iPEPS
Since many optimizers make separate calls to the objective function
and the gradient, but usually require both results for any given
parameter vector v, this function calls the gradient as well.
Args:
v: input variational parameters for the site tensors of
the iPEPS
Returns:
energy of the iPEPS at the point :attr:`v` in parameter space
"""
if self.cached_v is not None and np.linalg.norm(v - self.cached_v) < 1e-14:
return self.cached_out
else:
self.jac(v)
return self.cached_out
def check_grads(self, A=None):
print('Checking gradient')
self.peps.fill(A)
self.peps.converge_boundaries()
check_grads(self.peps.run, (A,), order=1, modes='rev')
print('Done check')


Fluidbox is a simple, lightweight but modern lightbox plugin written in javascript using jQuery and CSS3. Lightbox plugins are quite commonly used on modern websites to show users an image, multiple images or other content using a modal dialog.
Copyright (c) 2012 - 2013 Maarten de Boer -<EMAIL_ADDRESS>See the issues tracker for more coming features or post your own ideas!
Fluidbox has quite a few options you can change so here is a nice overview!
| Name | Values | Default | Description |
|---|---|---|---|
| animated | boolean |
true |
True to use animations if available, false to disable animations. |
| animations | false , PlainObject |
PlainObject |
Contains animation name for each action. |
| keys | PlainObject |
PlainObject |
Key codes for navigation actions |
| padding | integer |
50 |
Padding between the window borders and the image in pixels. |
| positions | PlainObject |
PlainObject |
Contains the positions for various Fluidbox elements. Eg. inner relates to #fluidbox-inner |
| preload | boolean |
true |
True to preload all images in collection instead of loading image when showed. |
| resize | boolean |
true |
True to center and resize overlay on window resize. |
| templates | PlainObject |
PlainObject |
Contains html templates of all Fluidbox elements. |
| touch | boolean |
true |
True to enable touchscreen support (when available), requires Hammer.js. |
* For all available animations for use in the animation
option, see http://daneden.me/animate/
To allow complete customization, Fluidbox triggers events to which you cand bind your own code to and do whatever you like!
See the Advanced Examples section in the menu for examples using these events
| Name | Arguments | Description |
|---|---|---|
fluidboxBeforeCreate |
Triggered before overlay and all other Fluidbox elements are created. | |
fluidboxAfterCreate |
Triggered after overlay and all other Fluidbox elements are created. | |
fluidboxBeforeBind |
Triggered before binding default keys and events. | |
fluidboxAfterBind |
Triggered after binding default keys and events. | |
fluidboxBeforeOpen |
Triggered before showing the overlay. | |
fluidboxAfterOpen |
Triggered after elements are created, keys are bound and the overlay is shown. Note: opening animation might still not be completed when this event is raised |
|
fluidboxBeforeShow |
index
target
direction
image
title
animation
|
Triggered before the new item is shown. |
fluidboxAfterShow |
Triggered after the new (next) item is shown. Note: prev/next animation might still not be completed when this event is raised |
|
fluidboxBeforeHide |
Triggered before the previously shown item is about to be cast into oblivion. | |
fluidboxAfterHide |
Triggered after the previously shown item is gone. Note: prev/next animation might still not be completed when this event is raised |
|
fluidboxBeforeClose |
Triggered when the overlay is about to close. | |
fluidboxAfterClose |
Triggered when the overlay is closed. Note: closing animation might still not be completed when this event is raised |
To get started: include jQuery, Fluidbox and optionally Modernizr and/or Hammer in the head
of your page like this:
<!DOCTYPE html>        <link rel="stylesheet" href="lib/css/animate.min.css">   <link rel="stylesheet" href="source/jquery.fluidbox.css">  ...
After that, include some images (or links to images) in your document to be used with fluidbox. Give them all a class
attribute, for example: 'fluidbox'. Optionally include a rel
attribute to group images into a gallery or leave it out to show a single image.
...   ...
or:
... Link to image 1 Link to image 2 ...
Last thing we need to do is initialize Fluidbox!
$(document).ready(function() { $('.fluidbox').fluidbox(); });
Simple demo demonstrating the use of fluidbox on single images, notice that no previous/next buttons are available. This is done by not giving the
element a rel
attribute.

$('.my-images').fluidbox();
Simple demo demonstrating the use of fluidbox on multiple images. You can browse through the images by using the previous/next buttons with your mouse, use the left/right arrow keys on your keyboard or if you have a touch device you can swipe with your finger.
To let fluidbox know your images belong together give the
a rel
attribute with a unique name, make sure they are all the same for all images!

$('.my-images').fluidbox();
Disabling buttons is easy, just set the button template to false
as demonstrated below. This is only a cosmetic change, you can still navigate through the images using your keyboard or touch device.
These button template options contain html, which means you can either change them or set them to false
to disable them. If you decide to change them, make sure you keep the ID
attribute the same.
Default ID's for buttons: next button: #fluidbox-btn-next
, previous button: #fluidbox-btn-prev
, close button: #fluidbox-btn-close
If you want to add more buttons or other elements you should modify the inner
, outer
or overlay
template instead, depending on where you want your element to appear.
$('.my-images').fluidbox({ templates: { buttons: { close: false, next: false, prev: false } } });
Titles are assigned to an image by using the title
attribute but you can add custom content to an image title by binding to the fluidboxBeforeShow
event.
$('.my-images').fluidbox().bind('fluidboxBeforeShow', function(event, item) { item.title += "- isn't it beautiful?"; });
You can specify custom animations per element by setting the animation
data attribute. The code below demonstrates this by specifying a custom prev/next animation for the first image.
$('.my-images').first().data('animation', { next: { in: 'rotateInDownRight', out: 'rotateOutUpLeft' }, prev: { in: 'rotateInDownLeft', out: 'rotateOutUpRight' } }); $('.my-images').fluidbox();
$('.my-images').fluidbox().bind('fluidboxBeforeShow', function(event, item) { if(item.index == 0) { item.animation = { next: { in: 'rotateInDownRight', out: 'rotateOutUpLeft' }, prev: { in: 'rotateInDownLeft', out: 'rotateOutUpRight' } }; } });


This simple example is great fun for friends and family alike! It contains multiple lines, because it does not conform to society's standards of beauty, but deep down it's looking to be accepted and is waiting for the right person to come along.


____ _ _________________________________________ \/ \ _/\ / \/ \ / oigtFit \/
VoigtFit¶
VoigtFit is written to make absorption line fitting a breeze. Dig in, and you will be constraining the contents of metals in remote galaxies before you know it!
Development of VoigtFit happens on GitHub so if you encounter any issues or you have ideas for great new features, you can raise an issue on the GitHub page.
Acknowledgements¶
If you use VoigtFit, please cite the description paper on arXiv (Krogager 2018).
I want to thank Jonatan Selsing and Kasper E. Heintz who helped putting parts of the documentation together. I also thank Svea Hernandez, Johan Fynbo, Christina Thöne, Luca Izzo, Antonio de Ugarte-Postigo, Bo Milvang-Jensen, and Lise Christensen for their help in extensively testing the software and for their constructive feedback and ideas for new features.
Recent updates¶
New in version 0.10.2:
Added support for LSF file format to specify the convolution kernel as a function of wavelength.
New in version 0.9.10:
Added two keywords to the parameter language in order to allow the user to view fit regions in velocity space when defining masks, continuum normalization and components. See details under sections Mask, Continuum Normalization and Interactive Components of the VoigtFit Parameter Language.
New in version 0.9.9:
New atomic data consistently gathered from the VALD database. The linelist has additional lines from Cashman et al. 2017 and for some lines not covered by VALD the damping constants have been taken from the compilation of Morton et al. 2003.
When masking lines, any predefined masks in the spectral data (loaded with the add_data statement) are now retained.
Installation instructions¶
Documentation¶
- VoigtFit Parameter Language
- Name
- Save
- z_sys
- Data
- Lines
- Fine-structure Lines
- Add Molecules
- Add Components
- Interactive Components
- Copy Components
- Delete Components
- Continuum Normalization
- Mask
- Clear mask
- Total Column Densities
- Metallicity
- Reset Fit Regions
- Resolution
- Change Systemic Redshift
- Thermal Model
- Fit-Options
- Output
- Load
- Fix Velocity Structure


About the site.
This site is hosted on the UCF Eustis server.
Thanks UCF for such a fast server.

I also want to mention that my site uses XHTML Strict 1.0 and validated the
first time I put it through the checker... no lie.
It took me about 2 hours to both prototype and code the header and the top
half of the main css sheet.
The biggest part of the site would have to be the header (including the nav bar). It's the most notable part of the site, and the hardest to develope.
The header uses a wrapper div to hold some more divs that contain all of those pretty links you see up there. The navbar is also up there (and the sub-navbar is inside of THAT wrapper). All in all, there are about 7 divs holding together the top of the page.
ON TOP OF THAT, I have another container class conveniently called "container" holding the entire page together and centering it on the screen (to a minimum of 900 pixels). So, as long as your screen is bigger than 12", the whole site'll be centered right in the middle of your screen!
The biggest part of the site would have to be the header (including the nav bar). It's the most notable part of the site, and the hardest to develope.
The header uses a wrapper div to hold some more divs that contain all of those pretty links you see up there. The navbar is also up there (and the sub-navbar is inside of THAT wrapper). All in all, there are about 7 divs holding together the top of the page.
ON TOP OF THAT, I have another container class conveniently called "container" holding the entire page together and centering it on the screen (to a minimum of 900 pixels). So, as long as your screen is bigger than 12", the whole site'll be centered right in the middle of your screen!
This site was developed using Google Chrome, Notepad++, and both Adobe Flash
and Adobe Photoshop. I also have to give credit to "The Consumerist" and "BBC",
both of whom have given me inspiration for my layout and design of this website.
I also want to say, if you're still using Firefox or Internet Explorer, you're
missing out. Google Chrome is wonderful. And it's faster than a Potato. More
on that here.
All pages on this site are valid under XHTML Strict 1.0. All CSS documents
are also valid under W3C's CSS validation.


Shibi (鴟尾) is an ornamental roof ornament used on the ridgepole, called oonume (大棟), of the tiled roof of a temple or palace.
They are also referred to as kutsugata (沓形) since the shape resembles a shoe.
Often, they are in the shape of a sachihoko (鯱鉾), an animal from Japanese folklore who's head is the shape of a tiger and it's body is the shape of a carp. The animal was believed to protect against fire and bring rain.
Traditionally, shibi were made from tile. They were later made from wood and covered in a copper shell. There are also a few stone shibi in existence.
— History
Historically, shibi were very popular in China, as well as during the Japanese Asuka and Hakuhou periods.


This check finds containers whose image contains known vulnerabilities.
- Where to find vulnerability reports?
-
Copy-paste the path part of the image (e.g.
"keppel.eu-de-1.cloud.sap/ccloud/limes") into your browser address bar. This
opens the image list for that repo in Elektra's Keppel UI. Find the relevant image
(look for a vulnerability status other than "Clean") and open its details
view to find the vulnerabilities, down near the image layers where they were
introduced.


About me
I can help you build a product, feature or website Look through some of my work and experience! If you like what you see and have a project you need coded, don’t hestiate to contact me.
Get my ResumeI can help you build a product, feature or website. Look through some of my work and experience! If you like what you see and have a project you need coded, don’t hestiate to contact me.
I can help you build a product, feature or website Look through some of my work and experience! If you like what you see and have a project you need coded, don’t hestiate to contact me.


const { slugify } = require(`../dependencies`);
module.exports = (workerPool, microserviceManifest) => {
return new Promise((resolve) => {
Arc loads resources it needs for microservice creation
const { slugify } = require(`../dependencies`);
module.exports = (workerPool, microserviceManifest) => {
return new Promise((resolve) => {
Given Arc gets the titles of the microservices from the manifest object
const titles = Object.keys(microserviceManifest);
When Arc creates microservices by their titles
const microservices = titles.map((unformattedTitle) => {
And Arc gets the manifest for the microservice
const manifest = microserviceManifest[unformattedTitle];
TODO: remove special characters from the microservice title
And Arc creates a slug from the microservice title
const title = slugify(String(unformattedTitle).toLocaleLowerCase());
Then Arc returns the microservice with the title
, manifest
and pool
set
return { title, manifest, pool: workerPool({title, manifest})};
});
Arc returns the microservices it created
resolve(microservices);
});
};


Sharks Forever
If you want to know about sharks, you're at the right place
Watch A Shark Swim
Footage of Another Shark
Shark Questions?
Contact a Shark


Information and services
The internet, television, phones, the arts and more.
News
Announcements, media releases, interviews, speeches and more.
-
Aged under 15: what does it mean for classifications?
-
nbn satellite service opens for business
-
2016 Prime Minister's Literary Awards now open
Our ministers
-
Minister for Communications
Senator the Hon Mitch Fifield


WITNESS LIST Insurance Committee February 11, 2003-10:00A HB 639 Committee Substitute (Smithee/CSHB 639) On: Floyd, Beaman (Tx Coaltion for Affordable Insurance Solutions (State Farm, Allstate, USAA, Nationwide, and AIA)) Schneider, Rob (Consumers Union)


nosh incorporates several interfaces and mechanisms that might be new to you:
Service and supervise directories are stored as two (of several) subdirectories of an over all service bundle directory. Other subdirectories contain symbolic links that define service interrelationships and orderings.
Bundle directories can live anywhere that one likes in the filesystem.
The system-control
program locates various standard targets in the /etc/service-bundles/targets
directory.
But those targets refer to other services (and targets) via symbolic links, which can point anywhere in the filesystem.
(A slight restriction on this is also the fairly obvious one:
Bundles for services and targets that are started in parallel with, or before, mounting the non-root filesystems must live on the root filesystem.
By convention, these "sysinit" bundles live in /etc/service-bundles/services
.
Since their supervise directories must be writable at run-time, they are symbolic links to directories that live under /run/service-bundles/early-supervise
.)
The service manager is not the system manager.
The service manager (service-manager
) manages dæmons, and their state transitions through the "stopped", "starting", "running", "failed", and "stopping" states.
The system manager (system-manager
) manages the state machine for the system as a whole, with the "normal", "rescue", and "emergency" bootstrap modes, the "halt", "reboot", and "poweroff" targets, and system-level control mechanisms such as hotkeys (Control+Alt+Delete and on Linux Alt-UpArrow) on the system console.
(Those familiar with Windows NT and ReactOS can see the system manager as akin to SMSS (the Session Manager Subsystem) which runs as process #1 and manages startup and shutdown, and the service manager as akin to SERVICES (the Service Controller) which manages service processes and provides an RPC API.
They are quite different when compared in detail, though.
Those familiar with IBM AIX can see the system manager as akin to init
and the service manager as akin to srcmstr
.
Similarly, those familiar with Solaris can see the system manager as akin to init
and the service manager as akin to svc.startd
.
Again, there are differences in the details.)
The service manager is not the service scanner.
In daemontools (and in
s6 and
daemontools-encore) the service scanner forks supervisory processes for services, directly.
In this system the daemontools-compatibility service scanner, service-dt-scanner
, talks through the RPC API to the service manager, which forks the service processes.
The service scanner is not the parent of service processes.
Indeed, it can be treated as a service itself (running under the service manager), and can be brought up and down.
Traditional daemontools service scanners are not expected to be terminated, in contrast.
One can do away with service-dt-scanner
and any /service/
directory entirely, moreover.
The service manager API provides mechanism; whereas tools like service-dt-scanner
determine in what particular way that mechanism is used, and are replaceable.
Running system-manager
as process #1, there's no daemontools-compatible scanner involved in normal operation.
Instead, system-control
institutes the full service/target bundle interdependency framework.
restart
scripts
Whenever the last service process for a service that is in the "running" state finishes, the service manager runs the service's restart
program.
(Some services, particularly targets, can be specially marked as "run on empty", which alters this behaviour.)
This program is given arguments that tell it the status of the last service process: whether it exited, crashed, aborted, was terminated, or was killed; and what the signal or exit code was.
A very simple restart
script executes the true
command, which causes the service to be unconditionally restarted by the service manager.
However, one can do a lot more than that.
More complex restart
scripts can …
… decide whether to restart or to stop dependent from how the process terminated;
… generate alert messages to monitoring systems;
… delay restarting services by pausing for some timeout interval;
… perform service-specific cleanup/reset actions.
This package has more standard targets than systemd, taking notions of distinct "multi-user" and "server" from the Solaris SMF milestones system:
Services that are part of running a workstation, as opposed to a server, machine are enabled by being added to the "wants" list of the standard "workstation" target.
Services that are part of running a server, as opposed to a workstation, machine are enabled by being added to the "wants" list of the standard "server" target.
Services that are part of providing multi-user login are enabled by being added to the "wants" list of the standard "multi-user" target.
It has different standard targets to systemd:
The default target is named "normal", not "default". "normal" encompasses "server", "workstation", "multi-user", "static-networking", and "users".
It also has fewer standard targets than systemd:
There are no "runlevel" targets. There is no concept of run-levels, full stop.


Filter District
district 1
Principal: Camille Wallin Address: 4862 BROADWAY, MANHATTAN NY 10034 Neighborhood: Marble Hill-Inwood Grades:0K,01,02,03,04,05Passed Math Exam (School):93%Passed Math Exam (District Average):40%
city
animal
space
SpaceX launches a Falcon 9 rocket from Cape Canaveral Air Force Station
space, nature
NASA Satellite view of Earth
A close up of a turtle underwater
nature
nature, city


| SfdcWebScrape | index /home/surf/sfdcexport/lib/SfdcWebScrape.py |
Class with methods to support logging into the salesforce.com website
in order to support operations that the sforce API does not yet support.
Author: Kevin Shuk<EMAIL_ADDRESS>Date: Mar 14, 2004
Copyright: (c) 2004 - 2005, Kevin Shuk and Magma Design Automation, Inc.
All Rights Reserved
| Modules | ||||||
|
| Classes | ||||||||
|
|
| Data | ||
| ident = '$ID: $' props = <Properties.Properties instance> |


|
HornetEngine
Open Alpha
Open source framework for creating Tangible Interfaces
|
Struct for storing Format Chunk data More...
Static Public Member Functions | |
| static FormatChunk | Parse (BinaryReader reader) |
| Tries to parse a format chunk from given stream More... | |
Public Attributes | |
| string | chunk_id |
| The id of this format chunk More... | |
| int | sub_chunk_size |
| The size of the format chunk More... | |
| short | audio_format |
| The format the audio is stored in (wave) More... | |
| short | num_channels |
| The amount of channels More... | |
| int | sample_rate |
| The sound sample rate in Hz More... | |
| int | byte_rate |
| The sound byte rate Bytes/Second More... | |
| short | block_align |
| short | bits_per_sample |
| The amount of bits per sound sample More... | |
Struct for storing Format Chunk data
|
static |
Tries to parse a format chunk from given stream
| reader | The binary reader to the opened audio file stream |
FormatChunk
///
| Exception |
| short HornetEngine.Sound.FormatChunk.audio_format |
The format the audio is stored in (wave)
| short HornetEngine.Sound.FormatChunk.bits_per_sample |
The amount of bits per sound sample
| short HornetEngine.Sound.FormatChunk.block_align |
| int HornetEngine.Sound.FormatChunk.byte_rate |
The sound byte rate Bytes/Second
| string HornetEngine.Sound.FormatChunk.chunk_id |
The id of this format chunk
| short HornetEngine.Sound.FormatChunk.num_channels |
The amount of channels
| int HornetEngine.Sound.FormatChunk.sample_rate |
The sound sample rate in Hz
| int HornetEngine.Sound.FormatChunk.sub_chunk_size |
The size of the format chunk


Pizza is my hero
Pizza is a combiantion of three basic ingredients: dough, sauce and cheese.
Pizza must contain:
peperoni
cheese
TOMATO SAUCE